Gamma-ray induced cascades in cosmic environments
- Autores
- Pellizza, Leonardo J.; Orellana, Mariana Dominga; Medina, María Clementina; Pedrosa, Susana E.; Romero, Gustavo Esteban; Tueros, Matías Jorge
- Año de publicación
- 2014
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- The new generation of gamma-ray telescopes has revealed a rich sky at very high photon energies. The unveiling of the nature of these sources and the understanding of the physical processes that give rise to the gammaray emission are among the most important present challenges of high-energy astrophysics. To investigate these issues, the propagation and interaction of the emitted electromagnetic radiation, both within the source and during its journey to the observer, must be understood. In this work we describe the development of a tool to provide an accurate, ab-initio description of the propagation of gamma rays in astrophysical environments. We expect this tool to contribute to the understanding of the physics of cosmic gamma-ray emitters.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
propagation of gamma rays
astrophysical environments
tool - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/165272
Ver los metadatos del registro completo
id |
SEDICI_d98d8b67e3b03a6baa247f61dca1fae2 |
---|---|
oai_identifier_str |
oai:sedici.unlp.edu.ar:10915/165272 |
network_acronym_str |
SEDICI |
repository_id_str |
1329 |
network_name_str |
SEDICI (UNLP) |
spelling |
Gamma-ray induced cascades in cosmic environmentsPellizza, Leonardo J.Orellana, Mariana DomingaMedina, María ClementinaPedrosa, Susana E.Romero, Gustavo EstebanTueros, Matías JorgeCiencias Astronómicaspropagation of gamma raysastrophysical environmentstoolThe new generation of gamma-ray telescopes has revealed a rich sky at very high photon energies. The unveiling of the nature of these sources and the understanding of the physical processes that give rise to the gammaray emission are among the most important present challenges of high-energy astrophysics. To investigate these issues, the propagation and interaction of the emitted electromagnetic radiation, both within the source and during its journey to the observer, must be understood. In this work we describe the development of a tool to provide an accurate, ab-initio description of the propagation of gamma rays in astrophysical environments. We expect this tool to contribute to the understanding of the physics of cosmic gamma-ray emitters.Facultad de Ciencias Astronómicas y Geofísicas2014-04info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf123-128http://sedici.unlp.edu.ar/handle/10915/165272enginfo:eu-repo/semantics/altIdentifier/isbn/978-987-24948-2-7info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:43:50Zoai:sedici.unlp.edu.ar:10915/165272Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:43:50.929SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Gamma-ray induced cascades in cosmic environments |
title |
Gamma-ray induced cascades in cosmic environments |
spellingShingle |
Gamma-ray induced cascades in cosmic environments Pellizza, Leonardo J. Ciencias Astronómicas propagation of gamma rays astrophysical environments tool |
title_short |
Gamma-ray induced cascades in cosmic environments |
title_full |
Gamma-ray induced cascades in cosmic environments |
title_fullStr |
Gamma-ray induced cascades in cosmic environments |
title_full_unstemmed |
Gamma-ray induced cascades in cosmic environments |
title_sort |
Gamma-ray induced cascades in cosmic environments |
dc.creator.none.fl_str_mv |
Pellizza, Leonardo J. Orellana, Mariana Dominga Medina, María Clementina Pedrosa, Susana E. Romero, Gustavo Esteban Tueros, Matías Jorge |
author |
Pellizza, Leonardo J. |
author_facet |
Pellizza, Leonardo J. Orellana, Mariana Dominga Medina, María Clementina Pedrosa, Susana E. Romero, Gustavo Esteban Tueros, Matías Jorge |
author_role |
author |
author2 |
Orellana, Mariana Dominga Medina, María Clementina Pedrosa, Susana E. Romero, Gustavo Esteban Tueros, Matías Jorge |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas propagation of gamma rays astrophysical environments tool |
topic |
Ciencias Astronómicas propagation of gamma rays astrophysical environments tool |
dc.description.none.fl_txt_mv |
The new generation of gamma-ray telescopes has revealed a rich sky at very high photon energies. The unveiling of the nature of these sources and the understanding of the physical processes that give rise to the gammaray emission are among the most important present challenges of high-energy astrophysics. To investigate these issues, the propagation and interaction of the emitted electromagnetic radiation, both within the source and during its journey to the observer, must be understood. In this work we describe the development of a tool to provide an accurate, ab-initio description of the propagation of gamma rays in astrophysical environments. We expect this tool to contribute to the understanding of the physics of cosmic gamma-ray emitters. Facultad de Ciencias Astronómicas y Geofísicas |
description |
The new generation of gamma-ray telescopes has revealed a rich sky at very high photon energies. The unveiling of the nature of these sources and the understanding of the physical processes that give rise to the gammaray emission are among the most important present challenges of high-energy astrophysics. To investigate these issues, the propagation and interaction of the emitted electromagnetic radiation, both within the source and during its journey to the observer, must be understood. In this work we describe the development of a tool to provide an accurate, ab-initio description of the propagation of gamma rays in astrophysical environments. We expect this tool to contribute to the understanding of the physics of cosmic gamma-ray emitters. |
publishDate |
2014 |
dc.date.none.fl_str_mv |
2014-04 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/conferenceObject info:eu-repo/semantics/publishedVersion Objeto de conferencia http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
format |
conferenceObject |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/165272 |
url |
http://sedici.unlp.edu.ar/handle/10915/165272 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/isbn/978-987-24948-2-7 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf 123-128 |
dc.source.none.fl_str_mv |
reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
reponame_str |
SEDICI (UNLP) |
collection |
SEDICI (UNLP) |
instname_str |
Universidad Nacional de La Plata |
instacron_str |
UNLP |
institution |
UNLP |
repository.name.fl_str_mv |
SEDICI (UNLP) - Universidad Nacional de La Plata |
repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
_version_ |
1844616306111807488 |
score |
13.070432 |